CCD Photometry and Lightcurve Analysis of Main Belt Asteroids 1077 Campanula and 1151 Ithaka from Observatori Carmelita

Details CCD Photometry and Lightcurve Analysis of Main Belt Asteroids 1077 Campanula and 1151 Ithaka from Observatori Carmelita CCD Photometry and Lightcurve Analysis of Main Belt Asteroids 1077 Campanula and 1151 Ithaka from Observatori Carmelita

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012mpbu...39...29a&link_type=abstract

The Minor Planet Bulletin (ISSN 1052-8091). Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Obse

Physics

Scientific paper

Observations carried out in 2011 August and September allowed us to
determine the synodic periods of 1077 Campanula and 1151 Ithaka. For
1077 Campanula, a period of 3.850 ± 0.001 h and amplitude of 0.36
mag were found. 1151 Ithaka exhibited an irregularly-shaped lightcurve
with a period of 4.932 ± 0.001 h and amplitude of 0.15 mag.

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